HIP 22051
HIP 22051 is a G-type (Yellow) star located in the constellation Perseus.
At a distance of roughly 1,977 light-years, HIP 22051 is a distant star lying deep within the Milky Way galaxy.
HIP 22051 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
At an apparent magnitude of +10.22, HIP 22051 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its yellow-white hue, which corresponds to a B-V color index of +0.753.
Physikalische Eigenschaften
| Spektralklasse | Class G — G-type (Yellow) |
| Farbindex (B−V) | 0,753 |
Beobachtung
| Scheinbare Helligkeit | +10.22 |
| Absolute Helligkeit | 1,31 |
| Entfernung | 1,977 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 4h 44,55m |
| Deklination | 42° 14,57′ |
Häufig gestellte Fragen
What type of star is HIP 22051?
HIP 22051 is a Class G — G-type (Yellow) star.
How far is HIP 22051 from Earth?
HIP 22051 is approximately 1,976.7 light-years from Earth.
Can you see HIP 22051 with the naked eye?
With an apparent magnitude of 10.22, HIP 22051 is not visible to the naked eye.
What constellation is HIP 22051 in?
HIP 22051 is located in the constellation Perseus.